AWAKE, the Advanced Proton Driven Plasma Wakefield Acceleration Experiment at CERN

Total Page:16

File Type:pdf, Size:1020Kb

AWAKE, the Advanced Proton Driven Plasma Wakefield Acceleration Experiment at CERN Nuclear Instruments and Methods in Physics Research A ∎ (∎∎∎∎) ∎∎∎–∎∎∎ Contents lists available at ScienceDirect Nuclear Instruments and Methods in Physics Research A journal homepage: www.elsevier.com/locate/nima AWAKE, The Advanced Proton Driven Plasma Wakefield Acceleration Experiment at CERN E. Gschwendtner b, E. Adli v, L. Amorim g, R. Apsimon c,j, R. Assmann e, A.-M. Bachmann l, F. Batsch l, J. Bauche b, V.K. Berglyd Olsen v, M. Bernardini b, R. Bingham o, B. Biskup b,d, T. Bohl b, C. Bracco b, P.N. Burrows i,w, G. Burt c, B. Buttenschön m, A. Butterworth b, A. Caldwell l, M. Cascella s, E. Chevallay b, S. Cipiccia x, H. Damerau b, L. Deacon s, P. Dirksen r, S. Doebert b, U. Dorda e, J. Farmer f, V. Fedosseev b, E. Feldbaumer b, R. Fiorito c,t, R. Fonseca g, F. Friebel b, A.A. Gorn a,n, O. Grulke m, J. Hansen b, C. Hessler b,W.Hofle b, J. Holloway i,w, M. Hüther l,q, D. Jaroszynski x, L. Jensen b, S. Jolly s, A. Joulaei l, M. Kasim i,w, F. Keeble s, Y. Li c,u, S. Liu r, N. Lopes h,g, K.V. Lotov a,n, S. Mandry s, R. Martorelli f, M. Martyanov l, S. Mazzoni b, O. Mete c,u, V.A. Minakov a,n, J. Mitchell c,j, J. Moody l, P. Muggli l, Z. Najmudin h,i, P. Norreys w,o,E.Özl, A. Pardons b, K. Pepitone b, A. Petrenko b, G. Plyushchev b,p, A. Pukhov f, K. Rieger l,q, H. Ruhl k, F. Salveter b, N. Savard l,r,y, J. Schmidt b, A. Seryi i,w, E. Shaposhnikova b, Z.M. Sheng x, P. Sherwood s, L. Silva g, L. Soby b, A.P. Sosedkin a,n, R.I. Spitsyn a,n, R. Trines o, P.V. Tuev a,n, M. Turner b, V. Verzilov r, J. Vieira g, H. Vincke b,Y.Weic,t, C.P. Welsch c,t, M. Wing s,e, G. Xia c,u, H. Zhang c,t a Budker Institute of Nuclear Physics SB RAS, Novosibirsk 630090, Russia b CERN, Geneva, Switzerland c Cockcroft Institute, Warrington WA4 4AD, UK d Czech Technical University, Zikova 1903/4, 166 36 Praha 6, Czech Republic e DESY, Notkestrasse 85, 22607 Hamburg, Germany f Heinrich-Heine-University of Düsseldorf, Moorenstrasse 5, Düsseldorf 40225, Germany g GoLP/Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, Lisbon, Portugal h John Adams Institute for Accelerator Science, Blackett Laboratory, Imperial College London, London SW7 2BW, UK i John Adams Institute for Accelerator Science, Oxford, UK j Lancaster University, Lancaster LA1 4YR, UK k Ludwig-Maximilians-Universität, Munich 80539, Germany l Max Planck Institute for Physics, Föhringer Ring 6, München 80805, Germany m Max Planck Institute for Plasma Physics, Wendelsteinstr. 1, Greifswald 17491, Germany n Novosibirsk State University, Novosibirsk 630090, Russia o STFC Rutherford Appleton Laboratory, Didcot OX11 0QX, UK p Swiss Plasma Center, EPFL, Lausanne 1015, Switzerland q Technische Universität München (TUM), Arcisstrasse 21, D-80333 Munich, Germany r TRIUMF, 4004 Wesbrook Mall, Vancouver V6T2A3, Canada s UCL, Gower Street, London WC1E 6BT, UK t University of Liverpool, Liverpool L69 7ZE, UK u University of Manchester, Manchester M13 9PL, UK v University of Oslo, Oslo 0316, Norway w University of Oxford, Oxford OX1 2JD, UK x University of Strathclyde, 16 Richmond Street, Glasgow G1 1XQ, UK y University of Victoria, 3800 Finnerty Rd, Victoria, Canada http://dx.doi.org/10.1016/j.nima.2016.02.026 0168-9002/& 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Please cite this article as: E. Gschwendtner, et al., Nuclear Instruments & Methods in Physics Research A (2016), http://dx.doi.org/ 10.1016/j.nima.2016.02.026i 2 E. Gschwendtner et al. / Nuclear Instruments and Methods in Physics Research A ∎ (∎∎∎∎) ∎∎∎–∎∎∎ article info abstract Article history: The Advanced Proton Driven Plasma Wakefield Acceleration Experiment (AWAKE) aims at studying Received 30 November 2015 plasma wakefield generation and electron acceleration driven by proton bunches. It is a proof-of- Received in revised form principle R&D experiment at CERN and the world's first proton driven plasma wakefield acceleration 5 February 2016 experiment. The AWAKE experiment will be installed in the former CNGS facility and uses the 400 GeV/c Accepted 9 February 2016 proton beam bunches from the SPS. The first experiments will focus on the self-modulation instability of the long (rms 12 cm) proton bunch in the plasma. These experiments are planned for the end of 2016. Keywords: Later, in 2017/2018, low energy (15 MeV) electrons will be externally injected into the sample wake- AWAKE fields and be accelerated beyond 1 GeV. The main goals of the experiment will be summarized. A Proton driven plasma wakefield accelera- summary of the AWAKE design and construction status will be presented. tion & 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license Linear accelerators Plasma wakefield (http://creativecommons.org/licenses/by/4.0/). Electron acceleration 1. Introduction transverse components of the plasma wakefields and the wake- fields being driven by regions of different bunch densities. The AWAKE is a proof-of-concept acceleration experiment with the modulation period sffiλpe and the modulated bunch resonantly aim to inform a design for high energy frontier particle accel- drives the plasma wakefields. The occurrence of the SMI can be erators and is currently being built at CERN [1,2]. The AWAKE detected by characterizing the longitudinal structure of the proton experiment is the world's first proton driven plasma wakefield beam when exiting the plasma cell. acceleration experiment, which will use a high-energy proton In the AWAKE master schedule, the experiment to obtain evi- bunch to drive a plasma wakefield for electron beam acceleration. dence for the SMI corresponds to Phase 1, and is expected to start A 400 GeV/c proton beam will be extracted from the CERN Super by the end of 2016. In Phase 2, AWAKE aims at the first demon- Proton Synchrotron, SPS, and utilized as a drive beam for wake- stration of proton-driven plasma wakefield acceleration of an fields in a 10 m long plasma cell to accelerate electrons with electron witness beam; this programme is planned to start by the amplitudes up to the GV/m level. Fig. 1 shows the AWAKE facility end of 2017. At a later phase it is foreseen to have two plasma cells in the CERN accelerator complex. In order to drive the plasma in order to separate the modulation of the proton bunch from the wakefields efficiently, the length of the drive bunch has to be on acceleration stage. Simulations [4] show that this would optimize λ the order of the plasma wavelength pe, which corresponds to the acceleration of external electrons and reach even higher E 14– 15 1 mm for the plasma density used in AWAKE (10 10 elec- gradients. trons/cm3). The proton beam for AWAKE has a bunch length of σ ¼ 12 cm, therefore the experiment relies on the self-modulation z 1.1. Baseline design instability (SMI) [3], which modulates the proton driver at the plasma wavelength in the first few meters of plasma. The SMI is a In the baseline design of AWAKE at CERN, an LHC-type proton transverse instability that arises from the interplay between bunch of 400 GeV/c (with an intensity of 3 Â 1011 protons/ bunch) will be extracted from the CERN SPS and sent along the 750 m long proton beam line towards a plasma cell. The AWAKE facility is installed in the area, which was previously used for the CERN Neutrinos to Gran Sasso facility (CNGS) [5]. The proton beam will be focused to σx;y ¼ 200 μm near the entrance of the 10 m long rubidium vapor plasma cell with an adjustable density in the 1014– 1015 electrons/cm3 range. When the proton bunch, with an r.m.s. bunch length of σz ¼ 12 cm (0.4 ns), enters the plasma cell, it undergoes the SMI. The effective length and period of the modu- lated beam is set by the plasma wavelength (for AWAKE, typically λpe ¼ 1 mm). A high power (E4.5 TW) laser pulse, co-propagating and co-axial with the proton beam, will be used to ionize the neutral gas in the plasma cell and also to generate the seed of the proton bunch self-modulation. An electron beam of 1:2 Â 109 electrons, which will be injected with 10–20 MeV/c into the plasma cell, serves as a witness beam and will be accelerated in the wake of the modulated proton bunch. Several diagnostic tools will be installed downstream of the plasma cell to measure the Fig. 1. CERN accelerator complex. proton bunch self-modulation effects and the accelerated electron Fig. 2. Baseline design of the AWAKE experiment. Please cite this article as: E. Gschwendtner, et al., Nuclear Instruments & Methods in Physics Research A (2016), http://dx.doi.org/ 10.1016/j.nima.2016.02.026i E. Gschwendtner et al. / Nuclear Instruments and Methods in Physics Research A ∎ (∎∎∎∎) ∎∎∎–∎∎∎ 3 Table 1 combination with a streak camera close to the plasma cell allow AWAKE proton, laser beam and plasma parameters. the overlap and synchronization of the beams to be measured. Optics simulations predict a 1σ spot size of 210 μm at the focal Parameter Baseline point in agreement with the experiment requirements (see Proton beam Table 1).
Recommended publications
  • CERN Courier–Digital Edition
    CERNMarch/April 2021 cerncourier.com COURIERReporting on international high-energy physics WELCOME CERN Courier – digital edition Welcome to the digital edition of the March/April 2021 issue of CERN Courier. Hadron colliders have contributed to a golden era of discovery in high-energy physics, hosting experiments that have enabled physicists to unearth the cornerstones of the Standard Model. This success story began 50 years ago with CERN’s Intersecting Storage Rings (featured on the cover of this issue) and culminated in the Large Hadron Collider (p38) – which has spawned thousands of papers in its first 10 years of operations alone (p47). It also bodes well for a potential future circular collider at CERN operating at a centre-of-mass energy of at least 100 TeV, a feasibility study for which is now in full swing. Even hadron colliders have their limits, however. To explore possible new physics at the highest energy scales, physicists are mounting a series of experiments to search for very weakly interacting “slim” particles that arise from extensions in the Standard Model (p25). Also celebrating a golden anniversary this year is the Institute for Nuclear Research in Moscow (p33), while, elsewhere in this issue: quantum sensors HADRON COLLIDERS target gravitational waves (p10); X-rays go behind the scenes of supernova 50 years of discovery 1987A (p12); a high-performance computing collaboration forms to handle the big-physics data onslaught (p22); Steven Weinberg talks about his latest work (p51); and much more. To sign up to the new-issue alert, please visit: http://comms.iop.org/k/iop/cerncourier To subscribe to the magazine, please visit: https://cerncourier.com/p/about-cern-courier EDITOR: MATTHEW CHALMERS, CERN DIGITAL EDITION CREATED BY IOP PUBLISHING ATLAS spots rare Higgs decay Weinberg on effective field theory Hunting for WISPs CCMarApr21_Cover_v1.indd 1 12/02/2021 09:24 CERNCOURIER www.
    [Show full text]
  • A Thermionic Electron Gun for the Preliminary Phase of Ctf3 G
    Proceedings of EPAC 2002, Paris, France A THERMIONIC ELECTRON GUN FOR THE PRELIMINARY PHASE OF CTF3 G. Bienvenu, M. Bernard, J. Le Duff, LAL, Orsay, France H. Hellgren, R. Pittin, L. Rinolfi, CERN, Geneva, Switzerland Abstract A dedicated electron gun has been designed and built Table 1: Beam parameters at gun exit for the preliminary phase of the CLIC Test Facility 3 Nominal beam energy 90 keV (CTF3). The gun is based on a thermionic gridded Pulse width 2 to 10 ns cathode and operates at 90 kV in the intensity range of Intensity 0.05 to 2 A 50 mA to 2A. The specific time structure of the beam is Number of pulses 1 to 7 characterized by a burst of up to seven pulses of variable Repetition rate 50 Hz pulse width (4 to 10 ns) each separated by 420 ns, the revolution time of the former EPA (Electron Positron Emittance (rms) <15 mm.mrd Accumulator) ring. The mechanical conception was specifically designed to be compatible with the existing 2.1 Mechanical design front-end of the former LIL (LEP Injector Linac). We will The vacuum chamber of the CLIO gun has been designed describe the experimental results obtained with the beam to fit existing CERN equipment, in particular the gun is on CTF3. fully compatible with the «CERN plug-in system» and an existing pair of ion pumps. All inner elements have been 1 INTRODUCTION baked under vacuum (400 ºC, 10-5 mbar, 12 h) and assembled under clean laminar airflow. With these The Compact Linear Collider (CLIC) scheme is based precautions a pressure of 10-9 mbar was obtained very on the production of a 30 GHz RF pulse that requires quickly and the HV processing reduced to a few hours.
    [Show full text]
  • CERN Celebrates Discoveries
    INTERNATIONAL JOURNAL OF HIGH-ENERGY PHYSICS CERN COURIER VOLUME 43 NUMBER 10 DECEMBER 2003 CERN celebrates discoveries NEW PARTICLES NETWORKS SPAIN Protons make pentaquarks p5 Measuring the digital divide pl7 Particle physics thrives p30 16 KPH impact 113 KPH impact series VISyN High Voltage Power Supplies When the objective is to measure the almost immeasurable, the VISyN-Series is the detector power supply of choice. These multi-output, card based high voltage power supplies are stable, predictable, and versatile. VISyN is now manufactured by Universal High Voltage, a world leader in high voltage power supplies, whose products are in use in every national laboratory. For worldwide sales and service, contact the VISyN product group at Universal High Voltage. Universal High Voltage Your High Voltage Power Partner 57 Commerce Drive, Brookfield CT 06804 USA « (203) 740-8555 • Fax (203) 740-9555 www.universalhv.com Covering current developments in high- energy physics and related fields worldwide CERN Courier (ISSN 0304-288X) is distributed to member state governments, institutes and laboratories affiliated with CERN, and to their personnel. It is published monthly, except for January and August, in English and French editions. The views expressed are CERN not necessarily those of the CERN management. Editor Christine Sutton CERN, 1211 Geneva 23, Switzerland E-mail: [email protected] Fax:+41 (22) 782 1906 Web: cerncourier.com COURIER Advisory Board R Landua (Chairman), P Sphicas, K Potter, E Lillest0l, C Detraz, H Hoffmann, R Bailey
    [Show full text]
  • A Spectrometer for Proton Driven Plasma Accelerated Electrons at Awake - Recent Developments∗
    Proceedings of IPAC2016, Busan, Korea WEPMY024 A SPECTROMETER FOR PROTON DRIVEN PLASMA ACCELERATED ELECTRONS AT AWAKE - RECENT DEVELOPMENTS∗ Lawrence Charles Deacon, Simon Jolly, Fearghus Keeble, UCL, London Aurélie Goldblatt, Stefano Mazzoni, Alexey Petrenko, CERN, Geneva Bartolomej Biskup, CERN, Geneva; Czech Technical University, Prague 6 Matthew Wing, UCL, London; DESY, Hamburg; University of Hamburg, Hamburg Abstract SPECTROMETER DESIGN The AWAKE experiment is to be constructed at the CERN Neutrinos to Gran Sasso facility (CNGS). This will be the first experiment to demonstrate proton-driven plasma wake- field acceleration. The 400 GeV proton beam from the CERN SPS will excite a wakefield in a plasma cell several meters in length. To probe the plasma wakefield, electrons of 10–20 MeV will be injected into the wakefield follow- ing the head of the proton beam. Simulations indicate that electrons will be accelerated to GeV energies by the plasma wakefield. The AWAKE spectrometer is intended to measure both the peak energy and energy spread of these accelerated electrons. Results of beam tests of the scintillator screen Figure 1: A 3D CAD image of the spectrometer system output are presented, along with tests of the resolution of annotated with distances along the z direction from the exit the proposed optical system. The results are used together of the plasma cell to the magnetic centers of magnets, and with a BDSIM simulation of the spectrometer system to pre- the center of the scintillator screen. dict the spectrometer performance for a range of possible accelerated electron distributions. INTRODUCTION RESOLUTION Proton bunches are the most promising drivers of wake- Optical System fields to accelerate electrons to the TeV energy scale in a The resolution of the energy spectrometer will ultimateley single stage.
    [Show full text]
  • Proton Driven Plasma Wakefield Acceleration in AWAKE
    Proton Driven Plasma Article submitted to journal Wakefield Acceleration in Subject Areas: AWAKE Plasma Wakefield Acceleration, 1 1 Proton Driven, Electron Acceleration E. Gschwendtner , M. Turner , **Author List Continues Next Page** Keywords: AWAKE, Plasma Wakefield Acceleration, Seeded Self Modulation In this article, we briefly summarize the experiments Author for correspondence: performed during the first Run of the Advanced Insert corresponding author name Wakefield Experiment, AWAKE, at CERN (European e-mail: [email protected] Organization for Nuclear Research). The final goal of AWAKE Run 1 (2013 - 2018) was to demonstrate that 10-20 MeV electrons can be accelerated to GeV- energies in a plasma wakefield driven by a highly- relativistic self-modulated proton bunch. We describe the experiment, outline the measurement concept and present first results. Last, we outline our plans for the future. 1 Continued Author List 2 E. Adli2,A. Ahuja1,O. Apsimon3;4,R. Apsimon3;4, A.-M. Bachmann1;5;6,F. Batsch1;5;6 C. Bracco1,F. Braunmüller5,S. Burger1,G. Burt7;4, B. Buttenschön8,A. Caldwell5,J. Chappell9, E. Chevallay1,M. Chung10,D. Cooke9,H. Damerau1, L.H. Deubner11,A. Dexter7;4,S. Doebert1, J. Farmer12, V.N. Fedosseev1,R. Fiorito13;4,R.A. Fonseca14,L. Garolfi1,S. Gessner1, B. Goddard1, I. Gorgisyan1,A.A. Gorn15;16,E. Granados1,O. Grulke8;17, A. Hartin9,A. Helm18, J.R. Henderson7;4,M. Hüther5, M. Ibison13;4,S. Jolly9,F. Keeble9,M.D. Kelisani1, S.-Y. Kim10, F. Kraus11,M. Krupa1, T. Lefevre1,Y. Li3;4,S. Liu19,N. Lopes18,K.V. Lotov15;16, M. Martyanov5, S.
    [Show full text]
  • A Time of Great Growth
    Newsletter | Spring 2019 A Time of Great Growth Heartfelt greetings from the UC Riverside Department of Physics and Astronomy. This is our annual newsletter, sent out each Spring to stay connected with our former students, retired faculty, and friends in the wider community. The Department continues to grow, not merely in size but also in stature and reputation. For the 2018-2019 academic year, we were pleased to welcome two new faculty: Professors Thomas Kuhlman and Barry Barish. Professor Kuhlman was previously on the faculty at the University of Illinois at Urbana-Champaign. He joins our efforts in the emerging field of biophysics. His research lies in the quantitative imaging and theoretical modeling of biological systems. He works on genome dynamics, quantification of the activity of transposable elements in living cells, and applications to the engineering of genome editing. Professor Barry Barish, who joins us from Caltech, is the winner of the 2017 Nobel Prize in Physics. He brings great prestige to our Department. Along with Professor Richard Schrock of the Department of Chemistry, who also joined UCR in 2018, UCR now has two Nobel Prize winners on its faculty. Professor Barish is an expert on the detection and physics of gravitational waves. He has been one of the key figures in the conception, construction, and operation of the LIGO detector, where gravitational waves were first discovered in 2015, and which led to his Nobel Prize. He is a member of the National Academy of Sciences and the winner of many other prestigious awards. The discovery of gravitational waves is one of the most exciting developments in physics so far this century.
    [Show full text]
  • The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland
    34th SLAC Summer Institute On Particle Physics (SSI 2006), July 17-28, 2006 The Large Hadron Collider Lyndon Evans CERN – European Organization for Nuclear Research, Geneva, Switzerland 1. INTRODUCTION The Large Hadron Collider (LHC) at CERN is now in its final installation and commissioning phase. It is a two-ring superconducting proton-proton collider housed in the 27 km tunnel previously constructed for the Large Electron Positron collider (LEP). It is designed to provide proton-proton collisions with unprecedented luminosity (1034cm-2.s-1) and a centre-of-mass energy of 14 TeV for the study of rare events such as the production of the Higgs particle if it exists. In order to reach the required energy in the existing tunnel, the dipoles must operate at 1.9 K in superfluid helium. In addition to p-p operation, the LHC will be able to collide heavy nuclei (Pb-Pb) with a centre-of-mass energy of 1150 TeV (2.76 TeV/u and 7 TeV per charge). By modifying the existing obsolete antiproton ring (LEAR) into an ion accumulator (LEIR) in which electron cooling is applied, the luminosity can reach 1027cm-2.s-1. The LHC presents many innovative features and a number of challenges which push the art of safely manipulating intense proton beams to extreme limits. The beams are injected into the LHC from the existing Super Proton Synchrotron (SPS) at an energy of 450 GeV. After the two rings are filled, the machine is ramped to its nominal energy of 7 TeV over about 28 minutes. In order to reach this energy, the dipole field must reach the unprecedented level for accelerator magnets of 8.3 T.
    [Show full text]
  • The AWAKE Acceleration Scheme for New Particle Physics Experiments at CERN
    AWAKE++: the AWAKE Acceleration Scheme for New Particle Physics Experiments at CERN W. Bartmann1, A. Caldwell2, M. Calviani1, J. Chappell3, P. Crivelli4, H. Damerau1, E. Depero4, S. Doebert1, J. Gall1, S. Gninenko5, B. Goddard1, D. Grenier1, E. Gschwendtner*1, Ch. Hessler1, A. Hartin3, F. Keeble3, J. Osborne1, A. Pardons1, A. Petrenko1, A. Scaachi3, and M. Wing3 1CERN, Geneva, Switzerland 2Max Planck Institute for Physics, Munich, Germany 3University College London, London, UK 4ETH Zürich, Switzerland 5INR Moscow, Russia 1 Abstract The AWAKE experiment reached all planned milestones during Run 1 (2016-18), notably the demon- stration of strong plasma wakes generated by proton beams and the acceleration of externally injected electrons to multi-GeV energy levels in the proton driven plasma wakefields. During Run 2 (2021 - 2024) AWAKE aims to demonstrate the scalability and the acceleration of elec- trons to high energies while maintaining the beam quality. Within the Physics Beyond Colliders (PBC) study AWAKE++ has explored the feasibility of the AWAKE acceleration scheme for new particle physics experiments at CERN. Assuming continued success of the AWAKE program, AWAKE will be in the position to use the AWAKE scheme for particle physics ap- plications such as fixed target experiments for dark photon searches and also for future electron-proton or electron-ion colliders. With strong support from the accelerator and high energy physics community, these experiments could be installed during CERN LS3; the integration and beam line design show the feasibility of a fixed target experiment in the AWAKE facility, downstream of the AWAKE experiment in the former CNGS area. The expected electrons on target for fixed target experiments exceeds the electrons on target by three to four orders of magnitude with respect to the current NA64 experiment, making it a very promising experiment in the search for new physics.
    [Show full text]
  • Status of the Ctf3 Commissioning
    Proceedings of EPAC 2002, Paris, France STATUS OF THE CTF3 COMMISSIONING R. Corsini, B. Dupuy, L. Rinolfi, P. Royer, F. Tecker, CERN, Geneva, Switzerland A. Ferrari∗, Uppsala University, Sweden Abstract In this paper, we describe the present status of the fa- cility as well as the results of the first beam measurements The Preliminary Phase of the new CLIC Test Facility performed during the commissioning [4, 5]. These results CTF3 consists of a low-charge demonstration of the elec- are compared to beam dynamics predictions [6]. Finally, tron bunch train combination process on which the CLIC the next steps towards the completion of the experiment drive beam generation scheme is based. The principle of are described. the combination relies on the injection of short electron bunches into an isochronous ring using RF deflecting cavi- ties. The commissioning of this facility started in Septem- 2 COMMISSIONING WITH BEAM ber 2001, with alternating periods of installation work and 2.1 The Front-End and the Linac beam studies. In this paper, we present the status of the facility, the first beam measurements and the next steps to- The new thermionic gun built by LAL (“Laboratoire wards the completion of the experiment. de l’Acc´el´erateur Lin´eaire d’Orsay”) was successfully in- stalled and commissioned [7]. This triode gun produces a train of up to seven pulses at a repetition rate of 50 Hz. The 1 INTRODUCTION pulse length can be varied between 2 ns and 10 ns FWHM and the pulses are spaced by 420 ns, corresponding to the The Compact Linear Collider (CLIC) [1] RF power revolution period of the ring, as required for the bunch fre- source scheme is based on the production of a 30 GHz quency multiplication process.
    [Show full text]
  • Barry Barish and the Gde: Mission Achievable
    INTERVIEW Barry Barish and the GDE: mission achievable The head of the Global Design Effort for a future International Linear Collider talks about challenges past, present and future. Barry Barish likes a challenge. He admits to a complete tendency to go for the difficult in his research – in his view, life is an adventure. Some might say that his most recent challenge would fit well with a certain famous TV series: “Your mission, should you choose to accept it… is to produce a design for the International Linear Collider that includes a detailed design concept, performance assessments, reliable international costing, an industrialization plan, and siting analysis, as well as detector concepts and scope.” Barish did indeed accept the challenge in March 2005, when he became director of the Global Design Effort (GDE) for a proposed International Linear Collider (ILC). He started in a directorate of one – himself – at the head of a “virtual” laboratory of hundreds of physicists and engineers around the globe. To run the “lab” he has set up a small executive committee, which includes three regional directors (for the Americas, Asia and Europe), three project manag- ers and two leading accelerator experts. There are also boards for R&D, change control and design cost. Barish operates from his base at Caltech, where he has been since 1962 and ultimately became Linde Professor of Physics (now emeri- tus). His taste for research challenges became evident in the 1970s, when he was co-spokesperson with Frank Sciulli (also at Caltech) of the “narrow band” neutrino experiment at Fermilab that studied Barish became director of the Global Design Effort for the International weak neutral currents and the quark substructure of the nucleon.
    [Show full text]
  • Gravitational Waves from the Early Universe
    Gravitational Waves from the Early Universe Lecture 1A: Gravitational Waves, Theory Kai Schmitz (CERN) Chung-Ang University, Seoul, South Korea j June 2 – 4 1/21 ◦ 1916: Albert Einstein predicts GWs based on his general theory of relativity ◦ 2016: The LIGO/Virgo Collaboration announces the detection of GW150914 ◦ 2017: Nobel Prize in Physics awarded to Rainer Weiss, Barry Barish, and Kip Thorne → Milestone in fundamental physics, triumph of general relativity → Discovery of a new class of astrophysical objects: heavy black holes in binary systems First direct detection of gravitational waves [Nicolle Rager Fuller for sciencenews.org] 2/21 ◦ 2016: The LIGO/Virgo Collaboration announces the detection of GW150914 ◦ 2017: Nobel Prize in Physics awarded to Rainer Weiss, Barry Barish, and Kip Thorne → Milestone in fundamental physics, triumph of general relativity → Discovery of a new class of astrophysical objects: heavy black holes in binary systems First direct detection of gravitational waves [Nicolle Rager Fuller for sciencenews.org] ◦ 1916: Albert Einstein predicts GWs based on his general theory of relativity 2/21 ◦ 2017: Nobel Prize in Physics awarded to Rainer Weiss, Barry Barish, and Kip Thorne → Milestone in fundamental physics, triumph of general relativity → Discovery of a new class of astrophysical objects: heavy black holes in binary systems First direct detection of gravitational waves [Nicolle Rager Fuller for sciencenews.org] ◦ 1916: Albert Einstein predicts GWs based on his general theory of relativity ◦ 2016: The LIGO/Virgo
    [Show full text]
  • Hep-Ph/0609102
    CERN-PH-TH/2006-175 September 2006 Physics Opportunities with Future Proton Accelerators at CERN A. Blondel a, L. Camilleri b, A. Ceccucci b, J. Ellis b , M. Lindroos b , M. Mangano b , G. Rolandi b a University of Geneva CH-1211 Geneva 4, SWITZERLAND b CERN, CH-1211 Geneva 23, SWITZERLAND Abstract We analyze the physics opportunities that would be made possible by upgrades of CERN’s proton accelerator complex. These include the new physics possible with luminosity or energy upgrades of the LHC, options for a possible future neutrino complex at CERN, and opportunities in other physics including rare kaon decays, other fixed-target experiments, nuclear physics and antiproton physics, among other possibilities. We stress the importance of inputs from initial LHC running and planned neutrino experiments, and summarize the principal detector R&D issues. 1 Introduction and summary In our previous report [1], we presented an initial survey of the physics opportunities that could be provided by possible developments and upgrades of the present CERN Proton Accelerator Complex [2,3]. These topics have subsequently been discussed by the CERN Council Strategy Group [4]. In this report, we amplify and update some physics points from our initial report and identify detector R&D priorities for the preferred experimental programme from 2010 onwards. We consider experimentation at the high-energy frontier to be the top priority in choosing a strategy for upgrading CERN's proton accelerator complex. This experimentation includes the upgrade to optimize the useful LHC luminosity integrated over the lifetime of the accelerator, through both a consolidation of the LHC injector chain and a possible luminosity upgrade project we term the SLHC.
    [Show full text]